{"as_of":"2026-08-16T14:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:70a3570093d20e8f8338f145dba152b674aeee06b4aadb6a34b961b26a79fd58","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":19,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":19,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":19,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":19,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T16:55:48.248799Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T12:28:08.032601Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-15T16:55:48.248799Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.19989","last_updated":"2025-08-27T15:48:09Z","snapshot_observed_at":"2026-08-16T12:38:33.706077Z","submitted_at":"2025-08-27T15:48:09Z","title":"Gravitational quasinormal modes of the Hayward spacetime","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T16:55:48.248799Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2508.19989"},"observation_digest":"sha256:86d4c02bf69169c2c7ae17306107d740194ea706fc075f680f631b2350aa087a","observation_id":"2f50eda7-f484-47b0-b074-3e9f4074a080","resolution":{"observed_at":"2026-08-15T16:55:48.248799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-15T15:48:38.310714Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.25141","last_updated":"2026-07-02T03:21:24Z","snapshot_observed_at":"2026-08-15T18:00:00.553943Z","submitted_at":"2025-09-29T17:51:18Z","title":"Quasinormal spectra of higher dimensional regular black holes in theories with infinite curvature corrections","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T15:48:38.310714Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2509.25141"},"observation_digest":"sha256:84813cbe5544d215f179e7c00b6b9270f7689d3496bb1cc1ce56f5b9b7011b77","observation_id":"67f61f8e-79e7-4c63-b8d9-11d9a67176cc","resolution":{"observed_at":"2026-08-15T15:48:38.310714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2510.11766","last_updated":"2026-03-30T15:33:50Z","snapshot_observed_at":"2026-07-31T11:31:52.166326Z","submitted_at":"2025-10-13T14:34:27Z","title":"Exact WKB method for radial Schr\\\"odinger equation","version":4},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-18T07:46:22.313894Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2510.11766"},"observation_digest":"sha256:2442255e6c78d0c7758d39e435a3ab8b83b5ea99766f352981cf92707fa1834a","observation_id":"90bc375c-c25b-4253-9e4f-47b0e594ccc5","resolution":{"observed_at":"2026-05-18T07:51:04.000367Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-03T20:15:07.131746Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.20778","last_updated":"2026-05-26T05:17:07Z","snapshot_observed_at":"2026-08-16T11:58:58.412157Z","submitted_at":"2025-11-25T19:16:21Z","title":"Exact WKB in all sectors II: Potentials with non-degenerate saddles","version":2},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-08-03T20:15:07.131746Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2511.20778"},"observation_digest":"sha256:a8c40025161a0935f372f2427fc423c3ac68d0cfa40e45e8fba388d6e17cc500","observation_id":"5d92e537-a27d-45d7-a0b7-d8fd1b4a37de","resolution":{"observed_at":"2026-08-03T20:15:07.131746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2512.17786","last_updated":"2026-05-04T11:04:58Z","snapshot_observed_at":"2026-08-12T20:30:50.967674Z","submitted_at":"2025-12-19T16:57:57Z","title":"Quasinormal modes of rotating black holes beyond general relativity in the WKB approximation","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-16T20:47:05.050295Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2512.17786"},"observation_digest":"sha256:f5e72cbbbd4a3e07c7c832bb2e898ad3c40a08d9f54b4ce7e32ec20e4eed8983","observation_id":"8d47895d-f7e7-4f53-8a18-d1d963623676","resolution":{"observed_at":"2026-05-16T20:48:32.530066Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-03T15:08:55.155275Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.18631","last_updated":"2026-06-03T12:09:17Z","snapshot_observed_at":"2026-08-16T02:23:15.578011Z","submitted_at":"2025-12-21T08:01:08Z","title":"Spectral instability of parametrized black hole quasinormal modes in the high-overtone limit via the exact WKB analysis","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T15:08:55.155275Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2512.18631"},"observation_digest":"sha256:3001531780a14d15c52f6db8a34cdbd8be3e934e030e44f19c8c9167b367dbde","observation_id":"e8614fa5-63ac-443c-ae3f-f8e337c731a5","resolution":{"observed_at":"2026-08-03T15:08:55.155275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-16T01:32:05.837925Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-21T14:22:03.468102Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:2b04040c0417970247909249276a4d378fdbd17f32cd08ad49d7bd5705b2a8c2","observation_id":"96973809-8e81-41aa-827c-9805a242d0ef","resolution":{"observed_at":"2026-05-21T14:24:13.475175Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-16T01:32:05.837925Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":3},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-25T07:20:50.943166Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:2c76bb1f8387893f446583254b1c9345397f25adb44b9902d47f321d0956b1d4","observation_id":"b93cbc2c-1865-44b1-bcb8-b30d770f3761","resolution":{"observed_at":"2026-05-25T07:25:29.859104Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2604.05878","last_updated":"2026-05-12T04:48:34Z","snapshot_observed_at":"2026-07-06T22:54:30.567988Z","submitted_at":"2026-04-07T13:39:17Z","title":"Exact WKB analysis of inverted triple-well: resonance, PT-symmetry breaking, and resurgence","version":1},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-05-10T19:31:50.995501Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2604.05878"},"observation_digest":"sha256:33f133d9e2767382c56ef57d977296df2850a2962797bee904dc90c5a0fcc331","observation_id":"3e7e5c5f-10a9-47e4-aa35-987d5f5358d3","resolution":{"observed_at":"2026-05-10T22:50:50.803832Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2604.05878","last_updated":"2026-05-12T04:48:34Z","snapshot_observed_at":"2026-07-06T22:54:30.567988Z","submitted_at":"2026-04-07T13:39:17Z","title":"Exact WKB analysis of inverted triple-well: resonance, PT-symmetry breaking, and resurgence","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-05-13T07:52:12.455546Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2604.05878"},"observation_digest":"sha256:976476be1dfdc0080cd993977d187fdec26fcdf5ee2196e83e8094e74956043c","observation_id":"8e3809ea-7f11-49d0-8a7a-86b981f2729b","resolution":{"observed_at":"2026-05-13T07:52:31.237482Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2604.20442","last_updated":"2026-08-06T06:11:02Z","snapshot_observed_at":"2026-08-09T23:09:40.603386Z","submitted_at":"2026-04-22T11:05:11Z","title":"Complex scaling approach to quasinormal modes of Schwarzschild and Reissner--Nordstr\\\"om black holes","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-10T00:16:02.497742Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2604.20442"},"observation_digest":"sha256:13d7655db85c7d5b18c6f9d28fba3983cd3910628548368f7015807db06404ad","observation_id":"a435040e-913f-406a-a26d-775ee901e1eb","resolution":{"observed_at":"2026-05-10T00:19:47.108455Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2605.01321","last_updated":"2026-05-02T08:38:13Z","snapshot_observed_at":"2026-07-06T23:14:33.653260Z","submitted_at":"2026-05-02T08:38:13Z","title":"Exact WKB and Quantum Periods for Extremal Black Hole Quasinormal Modes","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-09T15:05:51.457136Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2605.01321"},"observation_digest":"sha256:33f18058167b7007695ed84703c30eb77cc70457437999fae912a1533bc71109","observation_id":"445865ac-7cd7-41e6-aa36-557ada6ca11a","resolution":{"observed_at":"2026-05-11T16:46:07.210356Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2605.03277","last_updated":"2026-05-14T09:18:02Z","snapshot_observed_at":"2026-08-15T00:52:11.821396Z","submitted_at":"2026-05-05T02:09:06Z","title":"Quasinormal modes and continuum response of de Sitter black holes via complex scaling method","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-07T15:52:00.231481Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2605.03277"},"observation_digest":"sha256:0f17b0a8efd43631d50590d94be89f4deca90135de1f009a5f37995612598e13","observation_id":"92f1095d-91f9-4253-b949-8ff89ff7a892","resolution":{"observed_at":"2026-05-12T00:06:15.527798Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2605.03277","last_updated":"2026-05-14T09:18:02Z","snapshot_observed_at":"2026-08-15T00:52:11.821396Z","submitted_at":"2026-05-05T02:09:06Z","title":"Quasinormal modes and continuum response of de Sitter black holes via complex scaling method","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-15T07:19:22.926346Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2605.03277"},"observation_digest":"sha256:7d26bb3b2f2733c823ef75077338177ac063e3ce2db9d6ca48d31e7670383a39","observation_id":"0cb2abe5-7be7-48a0-8d60-e9fcb45d217e","resolution":{"observed_at":"2026-05-15T07:19:49.282232Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"2503.17245","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-03T12:28:08.032601Z","title":"Miyachi, R","venue":null,"work_id":"e1cf00b4-3e9f-45f9-ba6b-0632832d56ec","year":2025},"citing_paper":{"arxiv_id":"2606.12529","last_updated":"2026-07-20T13:34:40Z","snapshot_observed_at":"2026-08-16T04:18:28.086412Z","submitted_at":"2026-06-10T18:00:03Z","title":"Analytic approaches to perturbations of strongly coupled Yang-Mills plasma","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-06-27T08:57:44.309294Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2606.12529"},"observation_digest":"sha256:b9eb5864f7e1120c128872140acf71b263f298ea46f7db6882e852b5be1cb251","observation_id":"a27e3eb3-de64-4649-84d8-177399b3cdd3","resolution":{"observed_at":"2026-07-03T12:28:08.034192Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-02T11:51:36.475100Z","title":"Path to an exact WKB analysis of black hole quasinormal modes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.12529","last_updated":"2026-07-20T13:34:40Z","snapshot_observed_at":"2026-08-16T04:18:28.086412Z","submitted_at":"2026-06-10T18:00:03Z","title":"Analytic approaches to perturbations of strongly coupled Yang-Mills plasma","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-02T11:51:36.475100Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2606.12529"},"observation_digest":"sha256:2a490c206a7a5bf45cfe20143f913680631721c612d43e12490a8db86a90b601","observation_id":"c83dfabe-17fd-4c42-b91a-d315be1b03cf","resolution":{"observed_at":"2026-08-02T11:51:36.475100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-07-30T12:53:50.406571Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27043","last_updated":"2026-07-29T15:34:07Z","snapshot_observed_at":"2026-08-15T22:37:43.797666Z","submitted_at":"2026-07-29T15:34:07Z","title":"Resumming Kerr Quasinormal-Mode Frequencies: Accuracy and Breakdown Near Extremality","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-30T12:53:50.406571Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2607.27043"},"observation_digest":"sha256:6d9ced1ba8c389d8007ec7609e81b0fc2d5ef7953d71135f08329c36a504aed1","observation_id":"a4988880-0b6d-4b4f-beb5-6a6dbd96ab5a","resolution":{"observed_at":"2026-07-30T12:53:50.406571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-03T17:03:04.154555Z","title":"Miyachi, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28930","last_updated":"2026-07-31T01:18:01Z","snapshot_observed_at":"2026-08-15T05:25:59.352710Z","submitted_at":"2026-07-31T01:18:01Z","title":"Excitation region of Kerr black hole quasinormal modes from Stokes geometry","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T17:03:04.154555Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2607.28930"},"observation_digest":"sha256:2ed1fa4a0f6f134fef904e0453945669d83c02a64cd42ce6c877b8e395cb3a5e","observation_id":"4832ad8d-dd15-4ed4-b4cc-964fa919c5ce","resolution":{"observed_at":"2026-08-03T17:03:04.154555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17245","snapshot_observed_at":"2026-08-11T00:32:14.457863Z","title":"Path to an exact WKB analysis of black hole quasinormal modes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07678","last_updated":"2026-08-07T18:03:13Z","snapshot_observed_at":"2026-08-15T06:12:37.026430Z","submitted_at":"2026-08-07T18:03:13Z","title":"The Ringdown and the Tide: Fingerprints of Dark Matter Halo Profiles","version":1},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-08-11T00:32:14.457863Z"},"links":{"cited_paper":"/paper/2503.17245","citing_paper":"/paper/2608.07678"},"observation_digest":"sha256:d55a65bdc1631ce78594c188e94840560c9f6cbae403eb4567ba7fc2e436bed4","observation_id":"216aea06-b3d1-453c-8f5c-b3b46afcf89d","resolution":{"observed_at":"2026-08-11T00:32:14.457863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.17245/citation-record","integrity":"/paper/2503.17245/integrity","json":"/paper/2503.17245/citation-record.json","paper":"/paper/2503.17245"},"outbound":[],"paper":{"arxiv_id":"2503.17245","last_updated":"2025-07-09T06:46:17Z","latest_version":2,"primary_category":"hep-th","snapshot_observed_at":"2026-08-16T12:47:54.879572Z","submitted_at":"2025-03-21T15:50:59Z","title":"Path to an exact WKB analysis of black hole quasinormal modes"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2503.17245."}